Yakutsk EAS Array

Extensive Air Showers

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Intro to EAS

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In 1937 Schmeiser and Bothe pointed out that measurements of the Rossi transition curve (the frequency of coherent groups of particles vs. thickness of solid matter placed above the detector) always yield a positive intercept at zero thickness, and that this implies the occurrence of showers in the free air. Schmeiser & Bothe demonstrated that particles in the shower had separations up to at least 40 cm; but within a short time, Auger, Maze & Grivet-Meyer and Kolhorster, Matthes & Weber had measured coincidences between counters several tens of meters apart. The phenomena responsible for such coincidences have come to be known as extensive air showers, abbreviated as EAS…

The shower initiated by proton in lead plates of cloud chamber More recent investigations have verified that the frequency as a function of shower size is sufficient to permit practical measurements on events with primary energy up to at least 1017 eV. This fact accounts for the two principal motives for continued study of the EAS: to gather information related to the origin of the primary cosmic rays, and to investigate the nature of the interactions of extremely energetic particles.

The origin of the primary particles, the nature of any subsequent acceleration that they may experience, and the properties of the space in which they travel before reaching the earth determine several features of the local intensity that may be observable: the charge spectrum of the primaries; the shape of the energy spectrum; fluctuations of the intensity that may be correlated with disturbances on the sun or elsewhere outside the earth; and a possible asymmetry of the directional distribution in space, appearing as a periodic variation of the local intensity with solar or sidereal time owing to the rotation of the earth. In all of these respects, the primary rays that have extremely high energy, exceeding 1015 eV, may be expected to differ from much more abundant particles of comparatively low energy; and observation of the differences may shed light not only on the problem of the origin of cosmic rays but on various related astrophysical matters.

K. Greisen, The extensive air showers. Progress in cosmic ray physics, 1956,
North-Holland Publishing Co. Amsterdam, 3, 3.